activity
20162022
most citedThe Hot Companion and Circumbinary Disk of the Be Star HR 2142

54 citations · 158 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202232 cited

Dynamical masses of the primary Be star and the secondary sdB star in the single-lined binary kappa Dra (B6 IIIe)

R. Klement, D. Baade, Th. Rivinius +16

Because many classical Be stars may owe their nature to mass and angular-momentum transfer in a close binary, the present masses, temperatures, and radii of their components are of…

astro-ph.SR202222 cited

The statistical properties of early-type stars from LAMOST DR8

Yanjun Guo, Chao Liu, Luqian Wang +5

Massive binary stars play a crucial role in many astrophysical fields. Investigating the statistical properties of massive binary stars is essential to trace the formation of massi…

astro-ph.SR202217 cited

A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope

Jiangdan Li, Christopher A. Onken, Christian Wolf +12

Binaries consisting of a hot subdwarf star and an accreting white dwarf (WD) are sources of gravitational wave radiation at low frequencies and possible progenitors of type Ia supe…

astro-ph.SR202133 cited

Interferometric detections of sdO companions orbiting three classical Be stars

R. Klement, G. H. Schaefer, D. R. Gies +17

Classical Be stars are possible products of close binary evolution, in which the mass donor becomes a hot, stripped O or B-type subdwarf (sdO/sdB), and the mass gainer spins up and…

astro-ph.SR201654 cited

The Hot Companion and Circumbinary Disk of the Be Star HR 2142

Geraldine J. Peters, Luqian Wang, Douglas R. Gies +1

We present a spectroscopic investigation of the Be+sdO binary system HR 2142 that is based upon large sets of ultraviolet observations from the International Ultraviolet Explorer a…